Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2003-03-20
Phys.Rev. D68 (2003) 044003
Physics
High Energy Physics
High Energy Physics - Theory
14 pages with figures, version to appear in PRD
Scientific paper
10.1103/PhysRevD.68.044003
The search for regular black hole solutions in classical gravity leads us to consider a core of Euclidean signature in the interior of a black hole. Solutions of Lorentzian and Euclidean general relativity match in such a way that energy densities and pressures of an isotropic perfect fluid form are everywhere finite and continuous. Although the weak energy condition cannot be satisfied for these solutions in general relativity, it can be when higher derivative terms are added. A numerical study shows how the transition becomes smoother in theories with more derivatives. As an alternative to the Euclidean core, we also discuss a closely related time dependent orbifold construction with a smooth space-like boundary inside the horizon.
Hirayama Tadashi
Holdom Bob
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